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Analysis of resonant fast ion distributions during combined ICRF and NBI heating with transients using neutron emission spectroscopy

机译:使用中子发射光谱分析在瞬态ICRF和NBI联合加热过程中的共振快速离子分布

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摘要

This paper studies the deuterium distributions from 2nd harmonic ICRF heating at JET using neutron emission spectroscopy data from the time of flight spectrometer TOFOR. The fast deuterium distributions are obtained over the energy range 100 keV to 2 MeV. Specifically, we study how the how the fast deuterium distributions vary as ICRF heating is used alone as well as in combination with NBI heating. When comparing the different heating scenarios we observed both a difference in the slope of the distributions as well as in their absolute level. In the case of ICRF heating alone, the slope is Maxwellian-like over the entire energy range studied, while for the combined ICRF + NBI heating we observe a non-Maxwellian slope, which flattens out above 0.5 MeV . Comparisons are made with corresponding distributions calculated with the code PION. We find a good agreement between the measured distributions and those calculated with PION, both in terms of their shapes as well as their amplitudes. However, we also identified a period with an inverted fast ion distribution, which showed large disagreements between the modeled and measured results. Resonant interactions with tornado modes, i.e. core localized Toroidal Alfven Eigenmodes, are put forward as a likely explanation for the inverted distribution. 
机译:本文利用飞行时间谱仪TOFOR的中子发射光谱数据研究了JET二次谐波ICRF加热时的氘分布。快速氘分布是在100 keV至2 MeV的能量范围内获得的。具体来说,我们研究了单独使用ICRF加热以及与NBI加热结合使用时快速氘分布如何变化。当比较不同的供热方案时,我们观察到分布斜率及其绝对水平的差异。仅在ICRF加热的情况下,在研究的整个能量范围内,斜率都呈Maxwellian状,而对于ICRF + NBI组合加热,我们观察到非Maxwellian斜率,其平坦度超过0.5 MeV。与使用代码PION计算的相应分布进行比较。在形状和振幅方面,我们发现测得的分布与用PION计算的分布之间有很好的一致性。但是,我们还确定了一个快速离子分布反转的时期,这表明建模和测量结果之间存在很大分歧。提出了与龙卷风模式的共振相互作用,即核心局部环面阿尔文特征模式,作为对倒转分布的可能解释。

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